activity
19982026
most citedMasses of the Hyades white dwarfs: A gravitational redshift measurement

19 citations · 29 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2026

Wide binaries without viable bound Newtonian orbits

L. Pasquini, R. Saglia, F. Patat +7

Context. Wide binaries offer a unique opportunity to test gravity in the low acceleration regime, where deviations from Newtonian dynamics may appear. Aims. We use high-resolution…

astro-ph.GA2025★ 6 cited

Testing gravity with wide binaries -- 3D velocities and distances of wide binaries from Gaia and HARPS

R. Saglia, L. Pasquini, F. Patat +5

Wide Binaries (WBs) are interesting systems to test Newton-Einstein gravity in low potentials. The basic concept is to verify whether the difference in velocity between the WB comp…

astro-ph.SR2019★ 19 cited

Masses of the Hyades white dwarfs: A gravitational redshift measurement

L. Pasquini, A. F. Pala, H. -G. Ludwig +3

Context. It is possible to accurately measure the masses of the white dwarfs (WDs) in the Hyades cluster using gravitational redshift, because the radial velocity of the stars can…

astro-ph.IM2014★ 3 cited

Tachoastrometry: astrometry with radial velocities

L. Pasquini, C. Cortés, M. Lombardi +3

Spectra of composite systems (e.g., spectroscopic binaries) contain spatial information that can be retrieved by measuring the radial velocities (i.e., Doppler shifts) of the compo…

astro-ph1998★ 1 cited

Optical Identification of ROSAT sources in M 67: activity in an old cluster

L. Pasquini, T. Belloni

We present optical identification and high-resolution spectroscopy of ROSAT sources in the field of the old open cluster M 67. For the first time it is possible to analyze coronal…